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Fig. 10.
Gaussian fits to three strong emission lines in the last Keck spectrum. The [S II] λλ4069, 4076, [O I] λλ6300, 6364 and Hα profiles are here shown in common velocity space (the zero velocities correspond to 4068.6 Å, 6300.3 Å, and 6562.8 Å, respectively). The decompositions into Gaussians are tabulated in Table 4.
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